Non-LTE Inversions of the Mg II h & k and UV Triplet Lines
The Mg ii h & k lines are powerful diagnostics for studying the solar chromosphere. They have become particularly popular with the launch of the Interface Region Imaging Spectrograph (IRIS) satellite, and a number of studies that include these lines have lead to great progress in understanding chromospheric heating, in many cases thanks to the
de la Cruz Rodríguez, J. et al.
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2016